On the observability of T Tauri accretion shocks in the X-ray band

Astronomy and Astrophysics

Volumn 522, Issue 4, 2010, Pages

  Sacco, G G ^a,b   Orlando, S ^b   Argiroffi, C ^b,c   Maggio, A ^b   Peres, G ^b,c   Reale, F ^b,c   Curran, R L ^a,b  

^a ROCHESTER INSTITUTE OF TECHNOLOGY   (United States)

^b INAF OSSERVATORIO ASTROFISICO DI TORINO   (Italy)

^c UNIVERSITY OF PALERMO   (Italy)

Author keywords

accretion, accretion disks; hydrodynamics; shock waves; stars: pre main sequence; X rays: stars

Indexed keywords

ACCRETING MATERIALS; ACCRETION , ACCRETION DISKS; ACCRETION RATE; GRAVITY STRATIFICATION; HIGH DENSITY PLASMAS; HIGH RESOLUTION; HIGH VELOCITY; HYDRODYNAMIC MODEL; LOW DENSITY; MAGNETIC PRESSURE; METAL ABUNDANCES; MODEL RESULTS; QUASIPERIODIC OSCILLATIONS; RADIATIVE COOLING; RESONANCE LINE; SHOCK OSCILLATIONS; SOFT X-RAY; STAND OFF HEIGHT; STARS: PRE-MAIN SEQUENCE; STELLAR SURFACES; T TAURI STARS; THERMAL CONDUCTION; THERMAL INSTABILITIES; THERMAL PRESSURE; X RAY BANDS; X RAY DATA; X RAYS: STARS; X-RAY EMISSION; X-RAY OBSERVATIONS;

ABSORPTION; CHROMOPHORES; DISKS (MACHINE COMPONENTS); DISKS (STRUCTURAL COMPONENTS); FLUID DYNAMICS; HYDRAULICS; HYDRODYNAMICS; NEON; OBSERVABILITY; PLASMAS; SHOCK WAVES; STARS;

X RAYS;

EID: 78049461198     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201014950     Document Type: Article

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